Browsing by Author "Jones, P. A."

Now showing items 1-5 of 5

    • MALT90: The Millimetre Astronomy Legacy Team 90 GHz Survey 
      Jackson, J. M.; Rathborne, J.; Foster, J. B.; Whitake, J.; Sanhueza, P.; Claysmith, C.; Mascoop, J.; Wienen, M.; Breen, S.; Herpin, F.; Duarte Cabral, A.; Csengeri, T.; Longmore, S.; Contreras, Y.; Indermuehle, B.; Barnes, P.; Walsh, A. J.; Cunningham, M.; Brooks, K.; Britton, T.; Voronkov, M.; Urquhart, J.; Alves, J.; Jordan, C.; Hill, T.; Hoq, S.; Finn, S. C.; Bains, I.; Bontemps, S.; Bronfman Aguiló, Leonardo; Caswel, J.; Deharveng, L.; Ellingsen, S.; Fuller, G.; Garay Brignardello, Guido; Green, J.; Hindson, L.; Jones, P. A.; Lenfestey, C.; Lo, Nadia; Lowe, V.; Mardones Pérez, Diego; Menten, K.; Minier, V.; Morgan, L.; Motte, F.; Muller, E.; Peretto, N.; Purcell, C. R.; Schilke, P.; Bontemps, Schneider; Schuller, F.; Titmarsh, A.; Wyrowski, F.; Zavagno, A. (Astronomical Society of Australia, 2013)
      The Millimetre Astronomy Legacy Team 90 GHz (MALT90) survey aims to characterise the physical and chemical evolution of high-mass star-forming clumps. Exploiting the unique broad frequency range and on-the-fly ...
    • Spectral imaging of the Central Molecular Zone in multiple 3-mm molecular lines 
      Jones, P. A.; Burton, M. G.; Cunningham, M. R.; Requena Torres, M. A.; Menten, K. M.; Schilke, P.; Belloche, A.; Leurini, S.; Martín Pintado, J.; Ott, Jürgen; Walsh, A. J. (2012)
      We have mapped 20 spectral lines in the Central Molecular Zone (CMZ) around the Galactic Centre, emitting from 85.3 to 93.3 GHz. This work used the 22-m Mopra radio telescope in Australia, equipped with the 8-GHz bandwidth ...
    • Spectral imaging of the Sagittarius B2 region in multiple 7-mm molecular lines 
      Jones, P. A.; Burton, M. G.; Tothill, N. F. H.; Cunningham, M. R. (WILEY-BLACKWELL, 2011-03)
      We have undertaken a spectral-line imaging survey of a 6 x 6 arcmin2 area around Sagittarius (Sgr) B2 near the centre of the Galaxy, in the range from 30 to 50 GHz, using the Mopra telescope. The spatial resolution varies ...
    • Tracing H2 column density with atomic carbon (C i) and co isotopologs 
      Lo, Nadia; Cunningham, M. R.; Jones, P. A.; Bronfman Aguiló, Leonardo; Cortes, P. C.; Simon, R.; Lowe, V.; Fissel, L.; Novak, G. (2014-12-20)
      We present the first results of neutral carbon ([Ci] 3P1–3P0 at 492 GHz) and carbon monoxide (13CO, J = 1–0) mapping in the Vela Molecular Ridge cloud C (VMR-C) and the G333 giant molecular cloud complexes with the NANTEN2 ...
    • A view of Large Magellanic Cloud H II regions N159, N132, and N166 through the 345-GHz window 
      Paron, S.; Ortega, M. E.; Fariña, C.; Cunningham, M.; Jones, P. A.; Rubio López, Mónica (Oxford University Press, 2016)
      We present results obtained towards the H II regions N159, N166, and N132 from the emission of several molecular lines in the 345 GHz window. Using Atacama Submillimetre Telescope Experiment, we mapped a 2.4 arcmin x 2.4 ...